article Open AccessTop 1% cited
Gravitational-wave sensitivity curves
Classical and Quantum Gravity · 2014 · Vol. 32(1) · pp. 015014–015014
C. J. Moore✉(University of Cambridge)Robert H. Cole(University of Cambridge)C. P. L. Berry(University of Cambridge)
Abstract
There are several common conventions in use by the gravitational-wave community to describe the amplitude of sources and the sensitivity of detectors. These are frequently confused. We outline the merits of and differences between the various quantities used for parameterizing noise curves and characterizing gravitational-wave amplitudes. We conclude by producing plots that consistently compare different detectors. Similar figures can be generated on-line for general use at http://rhcole.com/apps/GWplotter.
Pulsars and Gravitational Waves ResearchAstrophysical Phenomena and ObservationsCosmology and Gravitation TheoriesPhysicsGravitational waveAmplitudeSensitivity (control systems)DetectorNoise (video)Gravitational-wave observatoryLine (geometry)GravitationAstrophysics
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